Radiation and Life
"Life on earth has developed with an ever present background of radiation.
It is not something new, invented by the wit of man: radiation has always been
there."
Eric J Hall, Professor of Radiology, College of Physicians and Surgeons,
Columbia University, New York, in his book "Radiation and Life".
Radiation and Life
Radiation is energy traveling through space. Sunshine is one of the most
familiar forms of radiation. It delivers light, heat and suntans. We control its
effect on us with sunglasses, shade, air conditioners, hats, clothes and
sunscreen.
There would be no life on earth without lots of sunlight, but we have
increasingly recognized that too much of it on our persons is not a good thing.
In fact it may be dangerous, so we control our exposure to it.
Sunshine consists of radiation in a range of wavelengths from long-wave
infra-red to short-wavelength ultraviolet, which creates the hazard.
Beyond ultraviolet are higher energy kinds of radiation which are used in
medicine and which we all get in low doses from space, from the air, and from
the earth. Collectively we can refer to these kinds of radiation as ionizing
radiation. It can cause damage to matter, particularly living tissue. At
high levels it is therefore dangerous, so it is necessary to control our
exposure.
Living things have evolved in an environment which has significant levels of
ionizing radiation. Furthermore, many of us owe our lives and health to such
radiation produced artificially. Medical and dental X-rays discern hidden
problems. Radiation is used to diagnose ailments, and some people are treated
with radiation to cure disease. We all benefit from a multitude of products and
services made possible by the careful use of radiation.
Background radiation is that which is naturally and inevitably present in our
environment. Levels of this can vary greatly. People living in granite areas or
on mineralized sands receive more terrestrial radiation than others, while
people living or working at high altitudes receive more cosmic radiation. A lot
of our natural exposure is due to radon, a gas which seeps from the earth's
crust and is present in the air we breathe.

European data from NRPB, Australian from ARPANSA.
THE UNSTABLE ATOM
Radiation comes from atoms, the basic building blocks of matter.
Most atoms are stable; a carbon-12 atom for example remains a carbon-12 atom
forever, and an oxygen-16 atom remains an oxygen-16 atom forever, but certain
atoms eventually disintegrate into a totally new atom. These atoms are said to
be 'unstable' or 'radioactive'. An unstable atom has excess internal energy,
with the result that the nucleus can undergo a spontaneous change towards a more
stable form. This is called 'radioactive decay'.
Each element exists in the form of atoms with several different sized nuclei,
called isotopes. Unstable isotopes (which are thus radioactive) are called
radioisotopes. Some elements, eg uranium, have no stable isotopes.
When an atom of a radioisotope decays, it gives off some of its excess energy
as radiation in the form of gamma rays or fast-moving sub-atomic particles. If
it decays with emission of an alpha or beta particle, it becomes a new element.
One can describe the emissions as gamma, beta and alpha radiation. All the time,
the atom is progressing in one or more steps towards a stable state where it is
no longer radioactive.
Another source of nuclear radioactivity is when one form of a radioisotope
changes into another form, or isomer, releasing a gamma ray in the process. The
excited form is signified with an "m" (meta) beside its atomic number, eg
technetium-99m (Tc-99m) decays to Tc-99. Gamma rays are often emitted with alpha
or beta radiation also, as the nucleus decays to a less excited state.
Apart from the normal measures of mass and volume, the amount of radioactive
material is given in Becquerel (Bq), a measure which enables us to
compare the typical radioactivity of some natural and other materials. A
Becquerel is one atomic decay per second *.
* A former unit of (radio)activity is the Curie - 1 Bq is 27 x
10-12 curies.
Radioactivity of some natural and other materials
| 1 adult human (100 Bq/kg) |
7000 Bq |
| 1 kg of coffee |
1000 Bq |
| 1 kg superphosphate fertiliser |
5000 Bq |
| The air in a 100 sq metre Australian home (radon) |
3000 Bq |
| The air in many 100 sq metre European homes (radon) |
30 000 Bq |
| 1 household smoke detector (with americium) |
30 000 Bq |
| Radioisotope for medical diagnosis |
70 million Bq |
| Radioisotope source for medical therapy |
100 000 000 million Bq |
| 1 kg 50-year old vitrified high-level nuclear waste |
10 000 000 million Bq |
| 1 luminous Exit sign (1970s) |
1 000 000 million Bq |
| 1 kg uranium |
25 million Bq |
| 1 kg uranium ore (Canadian, 15%) |
25 million Bq |
| 1 kg uranium ore (Australian, 0.3% |
)
500 000 Bq |
| 1 kg low level radioactive waste |
1 million Bq |
| 1 kg of coal ash |
2000 Bq |
| 1 kg of granite |
1000 Bq |
NB. Though the intrinsic radioactivity is the same, the
radiation dose received by someone handling a kilogram of high grade uranium ore
will be much greater than for the same exposure to a kilogram of separated
uranium, since the ore contains a number of short-lived decay products (see
section on Radioactive Decay).
RADIOACTIVE DECAY
Atoms in a radioactive substance decay in a random fashion but at a
characteristic rate. The length of time this takes, the number of steps required
and the kinds of radiation released at each step are well known.
The half-life is the time taken for half of the atoms of a radioactive
substance to decay. Half-lives can range from less than a millionth of a second
to millions of years depending on the element concerned. After one half-life the
level of radioactivity of a substance is halved, after two half-lives it is
reduced to one quarter, after three half-lives to one-eighth and so on.
All uranium atoms are mildly radioactive. The following figure for
uranium-238 shows the series of different radioisotopes it becomes as it decays,
the type of radiation given off at each step and the 'half-life' of each step on
the way to stable, non-radioactive lead-206. The shorter-lived each kind of
radioisotope, the more radiation it emits per unit mass. Much of the natural
radioactivity in rocks and soil comes from this decay chain.
see also ANSTO paper on
Radioactivity, Radioisotopes
etc
IONIZING RADIATION
Here we are concerned mainly with
ionizing radiation from the atomic nucleus. It occurs in two forms, rays and
particles, at the high frequency end of the energy spectrum.
Ionizing radiation produces electrically-charged particles called ions in the
materials it strikes. This process is called ionisation. In the large chemical
molecules of which all living things are made the changes caused may be
biologically important.
There are several types of ionizing radiation:

X-rays and gamma rays, like light, represent energy transmitted in a
wave without the movement of material, just as heat and light from a fire or the
sun travels through space. X-rays and gamma rays are virtually identical except
that X-rays are generally produced artificially rather than coming from the
atomic nucleus. Unlike light, X-rays and gamma rays have great penetrating power
and can pass through the human body. Thick barriers of concrete, lead or water
are used as protection from them.
Alpha particles consist of two protons and two neutrons, in the form
of atomic nuclei. They thus have a positive electrical charge and are emitted
from naturally occurring heavy elements such as uranium and radium, as well as
from some man-made elements. Because of their relatively large size, alpha
particles collide readily with matter and lose their energy quickly. They
therefore have little penetrating power and can be stopped by the first layer of
skin or a sheet of paper.
However, if alpha sources are taken into the body, for example by breathing
or swallowing radioactive dust, alpha particles can affect the body's cells.
Inside the body, because they give up their energy over a relatively short
distance, alpha particles can inflict more severe biological damage than other
radiations.
Beta particles are fast-moving electrons ejected from the nuclei of
atoms. These particles are much smaller than alpha particles and can penetrate
up to 1 to 2 centimeters of water or human flesh. Beta particles are emitted
from many radioactive elements. They can be stopped by a sheet of aluminum a few
millimeters thick.
Cosmic radiation consists of very energetic particles including
protons which bombard the earth from outer space. It is more intense at higher
altitudes than at sea level where the earth's atmosphere is most dense and gives
the greatest protection.
Neutrons are particles which are also very penetrating. On Earth they
mostly come from the splitting, or fissioning, of certain atoms inside a nuclear
reactor. Water and concrete are the most commonly used shields against neutron
radiation from the core of the nuclear reactor.
It is important to understand that alpha, beta, gamma and X-radiation does
not cause the body to become radioactive. However, most materials in their
natural state (including body tissue) contain measurable amounts of
radioactivity.
MEASURING IONIZING RADIATION
Grays and Sieverts
The human senses cannot detect radiation or discern whether a material is
radioactive. However, a variety of instruments can detect and measure radiation
reliably and accurately.
The amount of ionizing radiation, or 'dose', received by a person is measured
in terms of the energy absorbed in the body tissue, and is expressed in gray.
One gray (Gy) is one joule deposited per kilogram of mass.
Equal exposure to different types of radiation expressed as gray do not
however necessarily produce equal biological effects. One gray of alpha
radiation, for example, will have a greater effect than one gray of beta
radiation. When we talk about radiation effects, we therefore express the
radiation as effective dose, in a unit called the sievert (Sv).
Regardless of the type of radiation, one sievert (Sv) of radiation produces
the same biological effect.
Smaller quantities are expressed in 'millisievert' (one thousandth) or 'microsievert'
(one millionth) of a sievert. We will use the most common unit, millisievert
(mSv), here.
WHAT ARE THE HEALTH RISKS FROM IONIZING RADIATION?
It has been known for many years that large doses of ionizing radiation, very
much larger than background levels, can cause a measurable increase in cancers
and leukemias ('cancer of the blood') after some years delay. It must also be
assumed, because of experiments on plants and animals, that ionizing radiation
can also cause genetic mutations that affect future generations, although there
has been no evidence of radiation-induced mutation in humans. At very high
levels, radiation can cause sickness and death within weeks of exposure - see
Table.
The degree of damage caused by radiation depends on many factors Š dose, dose
rate, type of radiation, the part of the body exposed, age and health, for
example. Embryos including the human fetus are particularly sensitive to
radiation damage.
But what are the chances of developing cancer from low doses of radiation?
The prevailing assumption is that any dose of radiation, no matter how small,
involves a possibility of risk to human health. However there is no scientific
evidence of risk at doses below about 50 millisieverts in a short time or about
100 millisieverts per year. At lower doses and dose rates, up to at least 10
millisieverts per year, the evidence suggests that beneficial effects are as
likely as adverse ones.
Higher accumulated doses of radiation might produce a cancer which would only
be observed several - up to twenty - years after the radiation exposure. This
delay makes it impossible to say with any certainty which of many possible
agents were the cause of a particular cancer. In western countries, about a
quarter of people die from cancers, with smoking, dietary factors, genetic
factors and strong sunlight being among the main causes. Radiation is a weak
carcinogen, but undue exposure could certainly increase health risks.
The body has defense mechanisms against damage induced by radiation as well
as by chemical and other carcinogens. These can be stimulated by low levels of
exposure, or overwhelmed by very high levels.
On the other hand, large doses of radiation directed specifically at a tumor
are used in radiation therapy to kill cancerous cells, and thereby often save
lives (usually in conjunction with chemotherapy or surgery). Much larger doses
are used to kill harmful bacteria in food, and to sterilize bandages and other
medical equipment. Radiation has become a valuable tool in our modern world. See
also The Peaceful Atom in this
series.
Tens of thousands of people in each technically advanced country work in
medical and industrial environments where they may be exposed to radiation above
background levels. Accordingly they wear monitoring 'badges' while at work, and
their exposure is carefully monitored. The health records of these
occupationally exposed groups often show that they have lower rates of mortality
from cancer and other causes than the general public and, in some cases,
significantly lower rates than other workers who do similar work without being
exposed to radiation.
HOW MUCH IONIZING RADIATION IS DANGEROUS?
Radiation levels and their effects
The following table gives an indication of the likely effects of a range of
whole body radiation doses and dose rates to individuals:
10,000 mSv (10 sieverts) as
a short-term and whole-body dose would cause immediate illness, such as
nausea and decreased white blood cell count, and subsequent death within a
few weeks.
Between 2 and 10 sieverts in a short-term dose would cause severe radiation
sickness with increasing likelihood that this would be fatal. |
1,000 mSv (1 sievert) in a
short term dose is about the threshold for causing immediate radiation
sickness in a person of average physical attributes, but would be unlikely
to cause death. Above 1000 mSv, severity of illness increases with dose.
If doses greater than 1000 mSv occur over a long period they are less likely
to have early health effects but they create a definite risk that cancer
will develop many years later. |
| Above about 100 mSv, the probability of cancer
(rather than the severity of illness) increases with dose. The estimated
risk of fatal cancer is 5 of every 100 persons exposed to a dose of 1000 mSv
(ie. if the normal incidence of fatal cancer were 25%, this dose would
increase it to 30%). |
| 50 mSv is, conservatively,
the lowest dose at which there is any evidence of cancer being caused in
adults. It is also the highest dose which is allowed by regulation in any
one year of occupational exposure. Dose rates greater than 50 mSv/yr arise
from natural background levels in several parts of the world but do not
cause any discernible harm to local populations. |
| 20 mSv/yr averaged over 5
years is the limit for radiological personnel such as employees in the
nuclear industry, uranium or mineral sands miners and hospital workers (who
are all closely monitored). |
| 10 mSv/yr is the maximum
actual dose rate received by any Australian uranium miner. |
| 3-5 mSv/yr is the typical
dose rate (above background) received by uranium miners in Australia and
Canada. |
| 3 mSv/yr (approx) is the
typical background radiation from natural sources in North America,
including an average of almost 2 mSv/yr from radon in air. |
| 2 mSv/yr (approx) is the
typical background radiation from natural sources, including an average of
0.7 mSv/yr from radon in air. This is close to the minimum dose received by
all humans anywhere on Earth. |
| 0.3-0.6 mSv/yr is a typical
range of dose rates from artificial sources of radiation, mostly medical.
|
| 0.05 mSv/yr, a very small
fraction of natural background radiation, is the design target for maximum
radiation at the perimeter fence of a nuclear electricity generating
station. In practice the actual dose is less. |
BACKGROUND RADIATION
Naturally occurring background radiation is the main source of exposure for
most people. Levels typically range from about 1.5 to 3.5 millisievert per year
but can be more than 50 mSv/yr. The highest known level of background radiation
affecting a substantial population is in Kerala and Madras States in India where
some 140,000 people receive doses which average over 15 millisievert per year
from gamma radiation in addition to a similar dose from radon. Comparable levels
occur in Brazil and Sudan, with average exposures up to about 40 mSv/yr to many
people.
Several places are known in Iran, India and Europe where natural background
radiation gives an annual dose of more than 50 mSv and up to 260 mSv (at Ramsar
in Iran). Lifetime doses from natural radiation range up to several thousand
millisievert. However, there is no evidence of increased cancers or other health
problems arising from these high natural levels.
MAN-MADE RADIATION
Ionizing radiation is also generated in a range of medical, commercial and
industrial activities. The most familiar and, in national terms, the largest of
these sources of exposure is medical X-rays. A typical breakdown between natural
background and artificial sources of radiation is shown in the pie chart.
Natural radiation contributes about 88% of the annual dose to the population
and medical procedures most of the remaining 12%. Natural and artificial
radiations are not different in kind or effect.
PROTECTION FROM RADIATION
Because exposure to high levels of ionizing radiation carries a risk, should
we attempt to avoid it entirely? Even if we wanted to, this would be impossible.
Radiation has always been present in the environment and in our bodies. However,
we can and should minimize unnecessary exposure to significant levels of
man-made radiation.
Radiation is very easily detected. There is a range of simple, sensitive
instruments capable of detecting minute amounts of radiation from natural and
man-made sources. There are four ways in which people are protected from
identified radiation sources:
Limiting time: For people who are exposed to radiation in addition to
natural background radiation through their work, the dose is reduced and the
risk of illness essentially eliminated by limiting exposure time.
Distance: In the same way that heat from a fire is less the further
away you are, the intensity of radiation decreases with distance from its
source.
Shielding: Barriers of lead, concrete or water give good protection
from penetrating radiation such as gamma rays. Radioactive materials are
therefore often stored or handled under water, or by remote control in rooms
constructed of thick concrete or lined with lead.
Containment: Radioactive materials are confined and kept out of the
environment. Radioactive isotopes for medical use, for example, are dispensed in
closed handling facilities, while nuclear reactors operate within closed systems
with multiple barriers which keep the radioactive materials contained. Rooms
have a reduced air pressure so that any leaks occur into the room and not out
from the room.
STANDARDS AND REGULATION
Radiation protection standards are based on the conservative assumption
that the risk is directly proportional to the dose, even at the lowest levels,
though there is no evidence of risk at low levels. This assumption, called the
'linear no-threshold (LNT) hypothesis', is recommended for radiation protection
purposes only such as setting allowable levels of radiation exposure of
individuals. It cannot properly be used for predicting the consequences of an
actual exposure to low levels of radiation. For example, it suggests that, if
the dose is halved from a high level where effects have been observed, there
will be half the effect, and so on. This could be very misleading if applied to
a large group of people exposed to trivial levels of radiation and could lead to
inappropriate actions to avert the doses.
Much of the evidence which has led to today's standards derives from the
atomic bomb survivors in 1945, who were exposed to high doses incurred in a very
short time. In setting occupational risk estimates, some allowance has been made
for the body's ability to repair damage from small exposures, but for low-level
radiation exposure the degree of protection may be unduly conservative.
Most countries have their own systems of radiological protection which are
often based on the recommendations of the International Commission on
Radiological Protection (ICRP). The 'authority' of the ICRP comes from the
scientific standing of its members and the merit of its recommendations.
The three key points of the ICRP's recommendations are:
- Justification. No practice should be adopted unless its
introduction produces a positive net benefit.
- Optimization. All exposures should be kept as low as
reasonably achievable, economic and social factors being taken into account.
- Limitation. The exposure of individuals should not exceed
the limits recommended for the appropriate circumstances.
National radiation protection standards are based on ICRP recommendations for
both Occupational and Public exposure categories.
The ICRP recommends that the maximum permissible dose for occupational
exposure should be 20 millisievert per year averaged over five years (ie 100
millisievert in 5 years) with a maximum of 50 millisievert in any one year. For
public exposure, 1 millisievert per year averaged over five years is the
limit. In both categories, the figures are over and above background levels, and
exclude medical exposure.
In Australia, radiation protection regulations are set by States and
Territories, as well as by the Environment Protection (Nuclear Codes) Act 1978.
Two Codes of Practice have been developed to cover:
- Radiation Protection and Radioactive Waste Management in Mining and
Mineral Processing, 2002.
- Safe Transport of Radioactive Material, 2001.
Further information on the subject, together with links to overseas sources,
can be found in the briefing/information paper on
Radiation and the Nuclear Fuel Cycle.
The ARPANSA web site section on
Radiation and Health is
also valuable.
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